Under high strain rates, the effects of aluminum and vanadium on the deformation mechanisms of pure titanium have been revealed. However, the effect of oxygen, a prevalent interstitial element, remains less understood. In this study, we conducted dynamic uniaxial compressive loading on Ti-xO (x = 0.2, 0.4 wt%) polycrystals along the rolling direction (RD) using a split Hopkinson pressure bar (SHPB). Deformation mechanisms were analyzed via quasi-in-situ electron backscatter diffraction (EBSD) and slip trace analysis. The findings indicate that twinning and dislocation slip are significant in the Ti-0.2O polycrystal, with dislocation slip predominating in the Ti-0.4O polycrystal. Both polycrystals primarily activate {101‾2} tensile twins; however, twin nucleation and growth are markedly reduced in the Ti-0.4O polycrystal, a phenomenon associated with enhanced stacking fault energy (SFE) and oxygen segregation {101‾2} tensile twin boundaries. Unlike in quasi-static conditions, prismatic <a> slip is more probable in the Ti-0.4O polycrystal, while basal <a> slip, first-order pyramidal <a> slip, first-order pyramidal <c+a> slip, and second-order pyramidal <c+a> slip are inhibited to varying extents. These variations are attributed to increases in the ∣b<c+a>∣/∣b<a>∣ ratio, CRSSBasal<a>/CRSSPrismatic<a> ratio, and CRSSFirst-order pyramidal<a>/CRSSPrismatic<a> ratio with higher oxygen content. The Burgers vector is identified as more critical than the critical resolved shear stress (CRSS). Additionally, cross-slip between the <c+a> slip systems occurs in both polycrystals, facilitated by the complex core structure of the <c+a>-type dislocation. However, enhanced oxygen-dislocation interactions in the Ti-0.4O polycrystal result in reduced cross-slip planes.
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